An R band light curve for LP 71-82 showing flares, adapted from Baran et al. (2013) | |
Observation data Epoch J2000.0 Equinox J2000.0 | |
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Constellation | Draco |
Right ascension | 18 02 16.60 |
Declination | 64° 15′ 44.6″ |
Apparent magnitude (V) | 13.51 |
Characteristics | |
Spectral type | M5.0V |
Apparent magnitude (J) | 8.54 |
Astrometry | |
Proper motion (μ) | RA: 196.394 mas/yr Dec.: -383.789 mas/yr |
Parallax (π) | 128.3057 ± 0.0319 mas |
Distance | 25.420 ± 0.006 ly (7.794 ± 0.002 pc) |
Details | |
Mass | 0.16±0.01 M☉ |
Radius | 0.195±0.002 R☉ |
Luminosity | 0.0033±0.0003 L☉ |
Habitable zone inner limit | 0.06 |
Habitable zone outer limit | 0.12 |
Surface gravity (log g) | 4.5 cgs |
Temperature | 3124±51 K |
Rotation | 0.28018±0.000010 d |
Rotational velocity (v sin i) | 11.3±1.5 km/s |
Age | 0.5 −0.34 Gyr |
Other designations | |
Gaia DR2 2161121135533953536, G 227-22, LP 71-82, LSPM J1802+6415, NLTT 45873, GSC 04209-01465, 2MASS J18021660+6415445 | |
Database references | |
SIMBAD | data |
LP 71-82 is a red dwarf star, located in constellation Draco at 25.42 light-years from Earth. Kinematically, it is probably belongs to the Ursa Major Moving Group.
LP 71-82 is a flare star with a very strong activity, with at least four flares detected by 2019. Such activity is expected for a star with a short rotational period of just 6 hours. As a low mass star, it is fully convective. It is visible nearly pole-on, with rotational axis deflected from the Sun by 19±3° degrees. The star has a magnetic fields in chromosphere in 3.8-4.7 kilogauss range.
Multiplicity surveys did not find any stellar companions to LP 71-82 as in 2014.
References
- ^ Mt. Suhora Survey – Searching for Pulsating M Dwarfs. III
- Reiners, A.; et al. (2017), "The CARMENES search for exoplanets around M dwarfs", Astronomy & Astrophysics, 612: A49, arXiv:1711.06576, doi:10.1051/0004-6361/201732054
- ^ Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
- ^ Robertson, Paul; Stefansson, Gudmundur; Mahadevan, Suvrath; Endl, Michael; Cochran, William D.; Beard, Corey; Bender, Chad F.; Diddams, Scott A.; Duong, Nicholas; Ford, Eric B.; Fredrick, Connor; Halverson, Samuel; Hearty, Fred; Holcomb, Rae; Juan, Lydia; Kanodia, Shubham; Lubin, Jack; Metcalf, Andrew J.; Monson, Andrew; Ninan, Joe P.; Palafoutas, Jonathan; Ramsey, Lawrence W.; Roy, Arpita; Schwab, Christian; Terrien, Ryan C.; Wright, Jason T. (2020), "Persistent Starspot Signals on M Dwarfs: Multiwavelength Doppler Observations with the Habitable-zone Planet Finder and Keck/HIRES", The Astrophysical Journal, 897 (2): 125, arXiv:2005.09657, Bibcode:2020ApJ...897..125R, doi:10.3847/1538-4357/ab989f, S2CID 218718929
- ^ Rodríguez Martínez, Romy; Lopez, Laura A.; Shappee, Benjamin J.; Schmidt, Sarah J.; Jayasinghe, Tharindu; Kochanek, Christopher S.; Auchettl, Katie; Holoien, Thomas W.-S. (2019), "A Catalog of M-dwarf Flares with ASAS-SN", The Astrophysical Journal, 892 (2): 144, arXiv:1912.05549, doi:10.3847/1538-4357/ab793a, S2CID 209323915
- Reliable probabilistic determination of membership in stellar kinematic groups in the young disk, Table 4
- Shulyak, D.; Reiners, A.; Nagel, E.; Tal-Or, L.; Caballero, J. A.; Zechmeister, M.; Béjar, V. J. S.; Cortés-Contreras, M.; Martin, E. L.; Kaminski, A.; Ribas, I.; Quirrenbach, A.; Amado, P. J.; Anglada-Escudé, G.; Bauer, F. F.; Dreizler, S.; Guenther, E. W.; Henning, T.; Jeffers, S. V.; Kürster, M.; Lafarga, M.; Montes, D.; Morales, J. C.; Pedraz, S. (2019), "Magnetic fields in M dwarfs from the CARMENES survey", Astronomy & Astrophysics, 626: A86, arXiv:1904.12762, Bibcode:2019A&A...626A..86S, doi:10.1051/0004-6361/201935315, S2CID 139101130
- Janson, Markus; Bergfors, Carolina; Brandner, Wolfgang; Kudryavtseva, Natalia; Hormuth, Felix; Hippler, Stefan; Henning, Thomas (2014), "The Astralux Multiplicity Survey: Extension to Late M-Dwarfs", The Astrophysical Journal, 789 (2): 102, arXiv:1406.0535, Bibcode:2014ApJ...789..102J, doi:10.1088/0004-637X/789/2/102, S2CID 118403775
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